dc.contributor.author |
Moyssides, PG |
en |
dc.contributor.author |
Sarma, HNK |
en |
dc.contributor.author |
Carr, J |
en |
dc.contributor.author |
Debenham, NC |
en |
dc.contributor.author |
Garbutt, DA |
en |
dc.contributor.author |
Keyne, J |
en |
dc.date.accessioned |
2014-03-01T01:06:13Z |
|
dc.date.available |
2014-03-01T01:06:13Z |
|
dc.date.issued |
1983 |
en |
dc.identifier.issn |
0369-3546 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/9237 |
|
dc.subject |
14.40 |
en |
dc.subject |
Mesons and meson resonances |
en |
dc.subject.classification |
Physics, Particles & Fields |
en |
dc.title |
The problem of the X0-meson and its solution |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1007/BF02828984 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1007/BF02828984 |
en |
heal.language |
English |
en |
heal.publicationDate |
1983 |
en |
heal.abstract |
We fitted the X0 production cross-section data using a N* modulation to introduce a rise in the cross-section at low p *. The fit leads to several solutions, the best one being that having values for the parameters describing the Breit-Wigner resonance (E0,G{cyrillic}el, G{cyrillic}0) = (1889.3, 1.3-0.7+5.8, 1.2-0.9+9.2 ) MeV. Therefore, one can explain the behaviour of the X0 production cross-section in 7π~p scattering as being due to a narrow N* with mass near 1890 MeV and width ~ 2 MeV. © 1983 Società Italiana di Fisica. |
en |
heal.publisher |
Società Italiana di Fisica |
en |
heal.journalName |
Il Nuovo Cimento A |
en |
dc.identifier.doi |
10.1007/BF02828984 |
en |
dc.identifier.isi |
ISI:A1983QV36700003 |
en |
dc.identifier.volume |
75 |
en |
dc.identifier.issue |
2 |
en |
dc.identifier.spage |
163 |
en |
dc.identifier.epage |
172 |
en |